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Fig. 4


Evolutionary tracks in the radius-Teff plane for EI Cep. Solid lines denote models computed with STARS, while dashed lines denote models computed with MESA. Dark grey denotes the primary and light grey the secondary. The best fit STARS model is denoted with crosses, while the best fit MESA model is denoted with stars. The black errorbars denote the observed properties of the system.

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